JPL Technical Report Server

Performance sensitivity studies on the PIAA implementation of the high-contrast imaging testbed

Show simple item record

dc.contributor.author Sidick, Erkin
dc.contributor.author Lou, John Z.
dc.contributor.author Shaklan, Stuart
dc.contributor.author Levine, Marie
dc.date.accessioned 2015-05-14T23:18:26Z
dc.date.available 2015-05-14T23:18:26Z
dc.date.issued 2009-08-02
dc.identifier.citation SPIE Optics and Photonics, San Diego, California, August 2-6, 2009 en_US
dc.identifier.clearanceno 09-2572
dc.identifier.uri http://hdl.handle.net/2014/45181
dc.description.abstract We have investigated the dependence of the High Contrast Imaging Testbed (HCIT) Phase Induced Amplitude Apodization (PIAA) coronagraph system performance on the rigid-body perturbations of various optics. The structural design of the optical system as well as the parameters of various optical elements used in the analysis are drawn from those of the PIAA/HCIT system that have been and will be implemented, and the simulation takes into account the surface errors of various optics. In this paper, we report our findings when the input light is a narrowband beam. en_US
dc.description.sponsorship NASA/JPL en_US
dc.language.iso en_US en_US
dc.publisher Pasadena, CA : Jet Propulsion Laboratory, National Aeronautics and Space Administration, 2009 en_US
dc.subject Coronagraph en_US
dc.subject pupil mapping en_US
dc.subject exoplanets en_US
dc.title Performance sensitivity studies on the PIAA implementation of the high-contrast imaging testbed en_US
dc.type Preprint en_US


Files in this item

This item appears in the following Collection(s)

Show simple item record

Search


Browse

My Account